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Galactic Structure
Galactic Structure

...  Need to look closely at inhomogeneous chemical evolution models for dSph  Stars form in clusters/associations, natural?  Bulk of the stellar halo of the Milky Way does not look like the predictions from ΛCDM model so far.. ...
The Night Sky
The Night Sky

... We're two thirds of the way through fall, so Capella is shining in the northeast as soon as the stars come out. As night grows darker, look to its right by about three fists at arm's length for the frosty little Pleiades cluster. It's the size of your fingertip at arm's length. ...
Solar System Formation Reading
Solar System Formation Reading

... (1) (a) Most would agree that there is only one accurate description of the real solar system and that the real solar system followed one path of evolution. The question is whether we've figured it out or not. In the absence of complete knowledge about the past, can there be more than one theory tha ...
What makes stars tick?
What makes stars tick?

... by Liz Kruesi; illustrations by Roen Kelly ook up at the night sky from a dark site, and you’ll see tens of thousands of burning orbs of gas. Just one of those twinkling dots we call stars could be a behemoth with a mass 80 times that of our own Sun. At it’s core sits a cauldron of nuclear reactions ...
Chapter 10 Center of Gravity
Chapter 10 Center of Gravity

... A: Yes! A rigid object has one CG. If it is nonrigid, such as a piece of clay or putty, and is distorted into different shapes, then its CG may change as its shape is changed. Even then, it has one CG for any given shape. ...
Why Study Binary Stars?
Why Study Binary Stars?

... •  Doppler shift gives velocity of stars •  Blueshift for stars coming at us and •  Redshift for stars moving away ...
PPT - Lick Observatory
PPT - Lick Observatory

...  If stars were much farther away, then lack of detectable parallax was no longer so troubling. ...
A scenario of planet erosion by coronal radiation*
A scenario of planet erosion by coronal radiation*

... dependence of the erosion line on mass, combined with the mass distribution observed in Fig. 2, confirms that FX is the main variable, with few massive planets surviving exposure to high radiation as discussed below. The distribution of density with mass displayed in Fig. 3 is also consistent with t ...
Homework Assignment 2 Physics 55 Made available: Tuesday, September 6, 2005
Homework Assignment 2 Physics 55 Made available: Tuesday, September 6, 2005

... 2. In the Bohr model of the hydrogen atom, the electron acts like a planet that goes in a circular orbit around the proton, which then acts as the Sun (whose diameter is ≈ 109 m) . If the entire hydrogen atom were now magically magnified in size so that a proton had the same diameter as our Sun, wha ...
Million years - The Origin Of Life
Million years - The Origin Of Life

... takes just as long to rotate around its own axis as it does to revolve around its partner.”1 ...
Notes for Class 5, February 16
Notes for Class 5, February 16

... o Ptolemy (2nd cent AD) used new tools to simplify geocentric model of heavens • Epicycle (small sphere moved on larger sphere, planet on small sphere) • Eccentrics (circle displaced from earth) • Equant – point from which planet appeared to move at constant speed • Almagest – manual of Astronomy ...
The galaxies that host powerful radio sources
The galaxies that host powerful radio sources

... Angular resolution – comparable to the best optical imaging. No more “blobs at high redshift” – will be able to map the distribution of gas and dust in forming galaxies. ...
luminosities
luminosities

... With ground-based telescopes, we can measure parallaxes p ≥ 0.02 arc sec => d ≤ 50 pc ...
Senior thesis - University of Texas Astronomy Home Page
Senior thesis - University of Texas Astronomy Home Page

... up or down. In attempting to correct for this motion, this rising or sinking fluid will tend to “overshoot” its equilibrium point due to its own momentum. The small vertical oscillations caused by this process of a fluid constantly overshooting its equilibrium point will, in turn, create large horiz ...
Spectrum a Star….. - SFA Physics and Astronomy
Spectrum a Star….. - SFA Physics and Astronomy

... Spectrum a Star…..Day 1 ...
unit 23 - Institute for School Partnership
unit 23 - Institute for School Partnership

... Ask a student to hold the globe and another student hold the flashlight. Tell the class that the flashlight represents the sun and the globe the Earth. Have the “sun” and “Earth” stand in the middle of the room and have the “Earth” demonstrate the difference between revolve and rotate. Have the “Ear ...
Homework Assignment #7: The Moon
Homework Assignment #7: The Moon

... 2. The cause of the moon's phases: a. Where does the moon get its light from? b. What proportion of the moon is illuminated at any time? c. What phase is the moon in when it lies between the sun and the earth? Why? ...
HOU Supernova Light Curves
HOU Supernova Light Curves

... leaving nothing behind. The expanding cloud of ejecta glows brightly for many weeks as radioactive nickel produced in the explosion decays into cobalt and then iron. ...
Today`s Powerpoint
Today`s Powerpoint

... Emission Nebulae or H II Regions Regions of gas and dust near stars just formed. The Hydrogen is essentially fully ionized. Temperatures near 10,000 K Sizes about 1-20 pc. Hot tenuous gas => emission lines ...
Details of Emirates Mars Mission
Details of Emirates Mars Mission

... gravity, the probe will need to accelerate to an escape velocity of 39,000 km/h.   After around one minute, the first set of rocket boosters will detach and fall away,  followed by three more rocket stages which will fire up and fall away in turn until the  launcher releases the spacecraft onto its  ...
Venus will be too far north to transit the Sun.
Venus will be too far north to transit the Sun.

... Sec. R. S. N0 348, p.454. Translated from the Latin. It is well known that this distance of the sun from the earth, is supposed different by different astronomers. Ptolemy and his followers, as also Copernicus and Tycho Brahe, have computed it at 1200 semi-diameters of the earth, and Kepler at almos ...
Gizmos: H-R Diagrams
Gizmos: H-R Diagrams

... ________________________________________________ ...
Lecture 12
Lecture 12

... The light from the Andromeda galaxy left it about 1.5Myr ago, and the light from something in the Virgo Cluster about 65 Myr ago (about when the dinosaurs were killed). We’ll see we think the Universe is ~14Gyr old, so light from an object >14Glyr (5000Mpc) away will not have had enough time to reac ...
electron degeneracy pressure and white dwarfs
electron degeneracy pressure and white dwarfs

... Back to Chandrasekhar’s theory of white dwarfs  Important result of the theory: maximum mass for white dwarfs, which turns out to be 1.4 M. Electron degeneracy pressure cannot hold up a heavier mass.  Implication: for stars with core mass less than 1.4 M, core collapse is stopped by electron de ...
2-star-life-cycle-and-star-classification
2-star-life-cycle-and-star-classification

... 59. The star Algol is estimated to have approximately the same luminosity as the star Aldebaran approximately the same temperature as the Rigel. Algol is best classified as a A) main sequence star B) red giant star C) white dwarf star D) red dwarf star 60. Two stars of the same color are plotted on ...
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Timeline of astronomy

Timeline of astronomy around 2300 BC.
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